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MACRO absolute muon flux measurement: Comparison with Monte Carlo predictions

Authors :
Ambrosio M
Antolini R
Auriemma G
Baker R
Baldini A
Barbarino GC
Barish BC
Battistoni G
Bellotti R
Bemporad C
Bernardini P
Bilokon H
Bisi V
Bloise C
Bosio T
Bower C
Cafagna F
Calicchio M
Campana D
Carboni M
Castelliano M
Cecchini S
Cei F
Chiarella V
Corona A
Coutu S
DeCataldo G
Dekhissi R
DeMarzo C
DeMitri I
DeVincenzi M
DiCredico A
Erriquez O
Fantini R
Favuzzi C
Forti C
Fusco P
Giacomelli G
Giannini G
Giglietto N
Grassi M
Grillo A
Guarino F
Guarnaccia P
Gustavino C
Habig A
Hanson K
Hawthorne A
Heinz R
Hong JT
Iarocci E
Katsavounidis E
Kearns E
Kyriazopoulou S
Lamanna E
Lane C
Levin DS
Lipari P
Liu G
Liu R
Longley NP
Longo MJ
Lu Y
Ludlam G
Mancarella G
Mandrioli G
MargiottaNeri A
Marini A
Martello D
MarzariChiesa A
Mazziotta MN
Michael DG
Mikheyev S
Miller L
Mittelbrunn M
Monacelli P
Montaruli T
Monteno M
Mufson S
Musser J
Nicolo D
Nolty R
Okada C
Orth C
Osteria G
Palamara O
Parlati S
Patera V
Patrizii L
Pazzi R
Peck CW
Petrera S
Pignatano ND
Pistilli P
Popa V
Raino A
Reynoldson J
Ronga F
Rubizzo U
Sanzgiri A
Sartogo F
Satriano C
Satta L
Scapparone E
Scholberg K
Sciubba A
SerraLugaresi P
Severi M
Sitta M
Spada PF
Spinelli P
Spinetti M
Spurio M
Steinberg R
Stone JL
Sulak LR
Surdo A
Tarle G
Togo V
Valente V
Walter CW
Webb R.
BUSSINO, Severino Angelo Maria
Ambrosio, M
Antolini, R
Auriemma, G
Baker, R
Baldini, A
Barbarino, Gc
Barish, Bc
Battistoni, G
Bellotti, R
Bemporad, C
Bernardini, P
Bilokon, H
Bisi, V
Bloise, C
Bosio, T
Bower, C
Bussino, Severino Angelo Maria
Cafagna, F
Calicchio, M
Campana, D
Carboni, M
Castelliano, M
Cecchini, S
Cei, F
Chiarella, V
Corona, A
Coutu, S
Decataldo, G
Dekhissi, R
Demarzo, C
Demitri, I
Devincenzi, M
Dicredico, A
Erriquez, O
Fantini, R
Favuzzi, C
Forti, C
Fusco, P
Giacomelli, G
Giannini, G
Giglietto, N
Grassi, M
Grillo, A
Guarino, F
Guarnaccia, P
Gustavino, C
Habig, A
Hanson, K
Hawthorne, A
Heinz, R
Hong, Jt
Iarocci, E
Katsavounidis, E
Kearns, E
Kyriazopoulou, S
Lamanna, E
Lane, C
Levin, D
Lipari, P
Liu, G
Liu, R
Longley, Np
Longo, Mj
Lu, Y
Ludlam, G
Mancarella, G
Mandrioli, G
Margiottaneri, A
Marini, A
Martello, D
Marzarichiesa, A
Mazziotta, Mn
Michael, Dg
Mikheyev, S
Miller, L
Mittelbrunn, M
Monacelli, P
Montaruli, T
Monteno, M
Mufson, S
Musser, J
Nicolo, D
Nolty, R
Okada, C
Orth, C
Osteria, G
Palamara, O
Parlati, S
Patera, V
Patrizii, L
Pazzi, R
Peck, Cw
Petrera, S
Pignatano, Nd
Pistilli, P
Popa, V
Raino, A
Reynoldson, J
Ronga, F
Rubizzo, U
Sanzgiri, A
Sartogo, F
Satriano, C
Satta, L
Scapparone, E
Scholberg, K
Sciubba, A
Serralugaresi, P
Severi, M
Sitta, M
Spada, Pf
Spinelli, P
Spinetti, M
Spurio, M
Steinberg, R
Stone, Jl
Sulak, Lr
Surdo, A
Tarle, G
Togo, V
Valente, V
Walter, Cw
Webb, R.
Publication Year :
1995
Publisher :
ARGALIA EDITORE DELLE ARTI GRAFICHE EDITORIALI SRL, 1995.

Abstract

The vertical muon intensity measured with MACRO at the Gran Sasso Laboratory, in the depth range 3200-7000 hg cm(-2) of standard rock, corresponding to 2-200 TeV/nucleon primary energy range, is presented. An estimation of the muon energy spectrum at the surface will also be shown. The results will be compared with those of other experiments and with the computation of the intensities obtained using a full Monte Carlo calculation with different hypotheses for the primary cosmic ray composition.

Details

Language :
English
ISSN :
32007000
Database :
OpenAIRE
Accession number :
edsair.od......3668..219554a0196bf71bcf38dd1379781e11